Last modified: 05 June 1998 . Original version 05 June 1998 . ... If you have any questions regarding this schedule , please e-mail gensched@ vsop .isas.ac.jp or efomalon@nrao.edu VLBA V006e 0950+08 L Pent 328 Tu:Nov-24 15:00 - 02:00 S2 Percentage of time 7.7 HALCA Observations for WB = WESTERBORK EXPNO SOURCE FRQ Corr DOY DY: DATE UT RANGE Record/copy V090a2 3C309.1 L Socr 160 Tu:Jun-09 20:00 - 03:25 VLBA V050k 0454+844 C Socr 260 Th:Sep-17 04:00 - 11:00 VLBA V026b1 3C120 C ...

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Next: The Model Up: No Title Previous: Radiopulsars as Sources of . In this section, we study the evolution of stellar populations on a time-scale of 10 Myr for a starburst љ occurring under conditions similar to those in the Galactic Center (see Lipunov et al. (1995d)[ 126 ]). We estimate the expected number of X-ray transient љ sources (NS + MS star), super accreting BH, and BH + supergiant binaries, all as functions of time elapsed after the burst. ...

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